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Table 1

Observed properties of stars in our sample.

Star Prot Porb Teff [Fe/H] ρ⋆ f⊕ log (L⋆) Ref.
[d] [d] [K] [ρ⊙] [pW m-2] [L⊙]
55 Cnc 39.00 ± 9.00 0.74 5234 ± 30 +0.31 ± 0.04 120.4 ± 1.0 −0.244 ± 0.009 1, 2, 3, 4
CoRoT-2 4.52 ± 0.02 1.74 5598 ± 50 +0.04 ± 0.05 1.362 ± 0.064 5, 6
CoRoT-4 8.87 ± 1.12 9.20 6190 ± 60 +0.05 ± 0.07 7, 8
CoRoT-6 6.40 ± 0.50 8.89 6090 ± 70 −0.20 ± 0.10 0.929 ± 0.064 9, 8
CoRoT-7 23.64 ± 3.62 0.85 5313 ± 73 +0.03 ± 0.07 1.671 ± 0.073 10, 11, 12
CoRoT-13 4.04 5945 ± 90 +0.01 ± 0.07 0.526 ± 0.072 13, 8
CoRoT-18 5.40 ± 0.40 1.90 5440 ± 100 −0.10 ± 0.10 1.090 ± 0.160 14, 6
HAT-P-11 4.89 4780 ± 50 +0.31 ± 0.05 2.415 ± 0.097 5.9 ± 0.3 −0.590 ± 0.035 15, 8
HAT-P-21 15.90 ± 0.80 4.12 5634 ± 67 +0.04 ± 0.08 0.700 ± 0.150 16, 12
HATS-2 24.98 ± 0.04 1.35 5227 ± 95 +0.15 ± 0.05 1.220 ± 0.060 17, 17
HD 189733 11.95 ± 0.01 2.22 5050 ± 50 −0.03 ± 0.05 1.980 ± 0.170 27.5 ± 1.4 −0.489 ± 0.024 18, 19
HD 209458 10.65 ± 0.75 3.52 6117 ± 50 +0.02 ± 0.05 0.733 ± 0.008 23.1 ± 1.2 0.248 ± 0.041 20, 19
Kepler-17 12.10 ± 1.56 1.49 5781 ± 85 +0.26 ± 0.10 21, 6
Kepler-30 16.00 ± 0.40 29.33 5498 ± 54 +0.18 ± 0.27 1.420 ± 0.070 22, 23, 22
Kepler-63 5.40 ± 0.01 9.43 5576 ± 50 +0.05 ± 0.08 24, 24
Qatar-2 11.40 ± 0.50 1.34 4645 ± 50 −0.02 ± 0.08 1.591 ± 0.016 25, 25
WASP-4 22.20 ± 3.30 1.34 5540 ± 55 −0.03 ± 0.09 1.230 ± 0.022 26, 6
WASP-5 16.20 ± 0.40 1.63 5770 ± 65 +0.09 ± 0.09 0.801 ± 0.080 6
WASP-10 11.91 ± 0.05 3.09 4675 ± 100 +0.03 ± 0.20 27, 28, 29
WASP-19 11.76 ± 0.09 0.79 5460 ± 90 +0.14 ± 0.11 0.885 ± 0.006 30, 31
WASP-41 18.41 ± 0.05 3.05 5450 ± 150 −0.08 ± 0.09 1.270 ± 0.140 32, 32
WASP-46 16.00 ± 1.00 1.43 5600 ± 150 −0.37 ± 0.13 1.240 ± 0.100 33, 33
WASP-50 16.30 ± 0.50 1.96 5400 ± 100 −0.12 ± 0.08 1.376 ± 0.032 34, 35, 34
WASP-69 23.07 ± 0.16 3.87 4700 ± 50 +0.15 ± 0.08 1.540 ± 0.130 36, 36
WASP-77 15.40 ± 0.40 1.36 5500 ± 80 +0.00 ± 0.11 37, 37
WASP-84 14.36 ± 0.35 8.52 5300 ± 100 +0.00 ± 0.10 2.015 ± 0.070 36, 36
WASP-85 14.64 ± 1.47 2.66 5685 ± 65 +0.08 ± 0.10 1.280 ± 0.010 38, 38
WASP-89 20.20 ± 0.40 3.36 4960 ± 100 +0.15 ± 0.14 39, 39

Reference. (1) Henry et al. (2000); (2) Dragomir et al. (2014); (3) Valenti & Fischer (2005); (4) Boyajian et al. (2013); (5) Lanza et al. (2009); (6) Southworth (2012); (7) Aigrain et al. (2008); (8) Southworth (2011); (9) Fridlund et al. (2010); (10) Lanza et al. (2010); (11) Barros et al. (2014); (12) Torres et al. (2012); (13) Cabrera et al. (2010); (14) Hébrard et al. (2011); (15) Sanchis-Ojeda & Winn (2011); (16) Bakos et al. (2011); (17) Mohler-Fischer et al. (2013); (18) Henry & Winn (2008); (19) Southworth (2010); (20) Silva-Valio (2008); (21) Béky et al. (2014); (22) Sanchis-Ojeda et al. (2012); (23) Fabrycky et al. (2012); (24) Sanchis-Ojeda et al. (2013); (25) Mancini et al. (2014); (26) Sanchis-Ojeda et al. (2011); (27) Smith et al. (2009); (28) Christian et al. (2009); (29) Barros et al. (2013); (30) Tregloan-Reed et al. (2013); (31) Mancini et al. (2013); (32) Maxted et al. (2011); (33) Anderson et al. (2012); (34) Gillon et al. (2011); (35) Tregloan-Reed & Southworth (2013); (36) Anderson et al. (2014); (37) Maxted et al. (2013); (38) Brown et al. (2014); (39) Hellier et al. (2014).

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